SDO HMI 2014-11-11 06:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.99 | 0.00 | 11.16 | -10.80 | 337.26 | -23.40 | 121.70 | 0.4601 | -304.6 | -265.2 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.38 | 0.00 | 0.73 | -6.86 | 343.72 | -16.94 | 121.01 | 0.3390 | 718.0 | 533.7 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -9.78 | 342.89 | -17.77 | 126.63 | 0.3764 | 848.0 | 715.9 | |
| 0.00 | 2.07 | 0.00 | 1.14 | -13.18 | 340.17 | -20.49 | 129.41 | 0.4430 | 667.0 | 573.4 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -11.27 | 340.14 | -20.53 | 125.79 | 0.4257 | 680.0 | 571.8 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -12.32 | 337.03 | -23.63 | 124.04 | 0.4745 | -778.0 | -579.4 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -12.42 | 336.69 | -23.97 | 123.84 | 0.4797 | -734.0 | -542.4 | |
| 0.00 | 3.19 | 0.00 | 1.80 | -12.24 | 336.68 | -23.99 | 123.50 | 0.4784 | -787.0 | -670.5 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -10.16 | 336.40 | -24.26 | 119.37 | 0.4661 | -935.0 | -731.5 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -10.04 | 336.24 | -24.42 | 118.99 | 0.4674 | -977.0 | -782.9 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -10.39 | 335.52 | -25.15 | 118.96 | 0.4797 | -597.0 | -553.7 | |
| 0.00 | 3.27 | 0.00 | 1.87 | -10.91 | 334.53 | -26.13 | 118.98 | 0.4965 | -543.0 | -476.6 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -10.03 | 334.04 | -26.63 | 116.97 | 0.4972 | -778.0 | -612.7 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -6.95 | 332.49 | -28.18 | 110.06 | 0.5010 | -744.0 | -548.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |